In this review, we discuss the present status of three indirect techniques that are used to
determine reaction rates for stellar burning processes, asymptotic normalization coefficients …

X-ray binaries are among the brightest extra-solar objects in the sky and are characterized
by dramatic variabilities in brightness on timescales ranging from milliseconds to months …

We present results from the JINA REACLIB project, an ongoing effort to maintain a current
and accurate library of thermonuclear reaction rates for astrophysical applications. Ongoing …

A review of the evidence on the properties of the nuclei A= 8, 9 and 10, with emphasis on
material leading to information about the structure of the A= 8, 9, 10 systems.

Numerical values of charged-particle thermonuclear reaction rates for nuclei in the A= 14 to
40 region are tabulated. The results are obtained using a method, based on Monte Carlo …

The high resolution S800 spectrograph built at the National Superconducting Cyclotron
Laboratory (NSCL) is specially designed for reactions studies with radioactive beams. Its …

Isospin-symmetry breaking is responsible for the energy difference of excited states in mirror
nuclei. It also influences the coefficient of the isobaric multiplet mass equation. In the present …

Both one-proton and one-neutron knockout reactions were performed with fast beams of two
asymmetric, neutron-deficient rare isotopes produced by projectile fragmentation. The …

The nuclear physics input used to compute the Monte Carlo reaction rates and probability
density functions that are tabulated in the second paper of this series (Paper II) is presented …

The quest to comprehend how nuclear processes influence astrophysical phenomena is
driving experimental and theoretical research programs worldwide. One of the main goals in …